Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:


The Universe, Crisp and Clear

The next generation of adaptive optics has arrived at the Large Binocular Telescope in Arizona, providing astronomers with a new level of image sharpness surpassing that of the Hubble Space Telescope.

The next generation of adaptive optics has arrived at the Large Binocular Telescope in Arizona, providing astronomers with a new level of image sharpness never before seen.

Developed in a collaboration between Italy's Arcetri Observatory of the Istituto Nazionale di Astrofisica, or INAF, and the University of Arizona's Steward Observatory, this technology represents a remarkable step forward for astronomy.

"This is an incredibly exciting time as this new adaptive optics system allows us to achieve our potential as the world's most powerful optical telescope," said Richard Green, director of the LBT. "The successful results show that the next generation of astronomy has arrived, while providing a glimpse of the awesome potential the LBT will be capable of for years to come."

Until relatively recently, ground-based telescopes had to live with wavefront distortion caused by the Earth's atmosphere that significantly blurred the images of distant objects (this is why stars appear to twinkle to the human eye). While there have been advancements in adaptive optics technology to correct atmospheric blurring, the LBT's innovative system takes this concept to a new level.

This success was achieved through the combination of several innovative technologies. The first is the secondary mirror, which was designed from the start to be a main component of the LBT rather than an additional element as on other telescopes. The concave secondary mirror is .91 meters in diameter (3 feet) and only 1.6 millimeters thick.

The mirror is so thin and pliable that it can easily be manipulated by actuators pushing on 672 tiny magnets glued to the back of the mirror, which offers far greater flexibility and accuracy than previous systems on other telescopes. An innovative "pyramid" sensor detects atmospheric distortions and manipulates the mirror in real time to cancel out the blurring, allowing the telescope to literally see as clear as if there were no atmosphere.

Incredibly, the mirror is capable of making adjustments every one thousandth of a second, with accuracy to better than 10 nanometers (a nanometer is one millionth the size of a millimeter).

In closed-dome tests beginning May 12 and sky tests every night since May 25, astronomer Simone Esposito and his INAF team tested the new device, achieving exceptional results.

The LBT's adaptive optics system, called the First Light Adaptive Optics system, or FLAO, immediately outperformed all other comparable systems, delivering an image quality greater than three times sharper than the Hubble Space Telescope using just one of the LBT's two 8.4 meter mirrors. When the adaptive optics are in place for both mirrors and their light is combined appropriately, it is expected that the LBT will achieve image sharpness 10 times that of the Hubble.

The index of the perfection of image quality is known as the Strehl Ratio, with a ratio of 100 percent equivalent to an absolutely perfect image. Without adaptive optics, the ratio for ground-based telescopes is less than 1 percent. The adaptive optics systems on other major telescopes today improve image quality up to about 30 percent to 50 percent in the near-infrared wavelengths where the testing was conducted.

In the initial testing phase, the LBT's adaptive optics system has been able to achieve unprecedented Strehl Ratio of 60 to 80 percent, a nearly two-thirds improvement in image sharpness over other existing systems.

The results exceeded all expectations and were so precise the testing team had difficulty believing its findings. However, testing has continued since the system was first put on the sky on May 25, and the LBT's adaptive optics have functioned flawlessly and achieved peak Strehl Ratios of 82 to 84 percent.

"The results on the first night were so extraordinary that we thought it might be a fluke, but every night since the adaptive optics have continued to exceed all expectations. These results were achieved using only one of LBT's mirrors. Imagine the potential when we have adaptive optics on both of LBT's giant eyes," Esposito said.

More images from the adaptive optics system are available at the LBT Observatory website.

Development of the LBT's adaptive optics system took longer than a decade through an international collaboration. INAF, in particular the Arcetri Observatory, conceived the instrument design and developed the electro-mechanical system, while the University of Arizona Mirror Lab created the optical elements, and the Italian companies Microgate and ADS International engineered several components.

A prototype system was previously installed on the Multiple Mirror Telescope, or MMT, at Mt. Hopkins, Ariz. The MMT system uses roughly half the number of actuators as the LBT's final version, but it demonstrated the viability of the design. The LBT's infrared test camera, which produced the accompanying images, was a joint development of INAF in Bologna and the MPIA in Heidelberg.

"This has been a tremendous success for INAF and all of the partners in the LBT," said Piero Salinari, research director at the Arcetri Observatory, INAF. "After more than a decade and with so much care and effort having gone into this project, it is really rewarding to see it succeed so astoundingly."

The $120 million LBT on Mount Graham utilizes two giant 8.4 meter mirrors and with the new adaptive optics the telescope will have the resolution of a 22.8-meter, or approximately 75-foot telescope. The new adaptive optics will enable versatile instruments such as the near-infrared camera spectrometer, which allows astronomers to penetrate interstellar dust clouds and reveal the secrets of the youngest and most distant galaxies, to achieve their full potential on the LBT.

The LBT is an international collaboration among institutions in the U.S., Italy and Germany. The LBT Corporation partners are:

The University of Arizona on behalf of the Arizona university system

Istituto Nazionale di Astrofisica, Italy
LBT Beteiligungsgesellschaft, Germany, representing the Max Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University

The Ohio State University
The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota and University of Virginia
Richard Green, Large Binocular Telescope Observatory
Jennifer Fitzenberger, University Communications

Jennifer Fitzenberger | University of Arizona
Further information:

More articles from Physics and Astronomy:

nachricht Gamma ray camera offers new view on ultra-high energy electrons in plasma
28.10.2016 | American Physical Society

nachricht Scientists measure how ions bombard fusion device walls
28.10.2016 | American Physical Society

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: Novel light sources made of 2D materials

Physicists from the University of Würzburg have designed a light source that emits photon pairs. Two-photon sources are particularly well suited for tap-proof data encryption. The experiment's key ingredients: a semiconductor crystal and some sticky tape.

So-called monolayers are at the heart of the research activities. These "super materials" (as the prestigious science magazine "Nature" puts it) have been...

Im Focus: Etching Microstructures with Lasers

Ultrafast lasers have introduced new possibilities in engraving ultrafine structures, and scientists are now also investigating how to use them to etch microstructures into thin glass. There are possible applications in analytics (lab on a chip) and especially in electronics and the consumer sector, where great interest has been shown.

This new method was born of a surprising phenomenon: irradiating glass in a particular way with an ultrafast laser has the effect of making the glass up to a...

Im Focus: Light-driven atomic rotations excite magnetic waves

Terahertz excitation of selected crystal vibrations leads to an effective magnetic field that drives coherent spin motion

Controlling functional properties by light is one of the grand goals in modern condensed matter physics and materials science. A new study now demonstrates how...

Im Focus: New 3-D wiring technique brings scalable quantum computers closer to reality

Researchers from the Institute for Quantum Computing (IQC) at the University of Waterloo led the development of a new extensible wiring technique capable of controlling superconducting quantum bits, representing a significant step towards to the realization of a scalable quantum computer.

"The quantum socket is a wiring method that uses three-dimensional wires based on spring-loaded pins to address individual qubits," said Jeremy Béjanin, a PhD...

Im Focus: Scientists develop a semiconductor nanocomposite material that moves in response to light

In a paper in Scientific Reports, a research team at Worcester Polytechnic Institute describes a novel light-activated phenomenon that could become the basis for applications as diverse as microscopic robotic grippers and more efficient solar cells.

A research team at Worcester Polytechnic Institute (WPI) has developed a revolutionary, light-activated semiconductor nanocomposite material that can be used...

All Focus news of the innovation-report >>>



Event News

#IC2S2: When Social Science meets Computer Science - GESIS will host the IC2S2 conference 2017

14.10.2016 | Event News

Agricultural Trade Developments and Potentials in Central Asia and the South Caucasus

14.10.2016 | Event News

World Health Summit – Day Three: A Call to Action

12.10.2016 | Event News

Latest News

Prototype device for measuring graphene-based electromagnetic radiation created

28.10.2016 | Power and Electrical Engineering

Gamma ray camera offers new view on ultra-high energy electrons in plasma

28.10.2016 | Physics and Astronomy

When fat cells change their colour

28.10.2016 | Life Sciences

More VideoLinks >>>